In recent studies to understand the nature of the universe, a new DE model has been constructed
in the context of quantum gravity on holographic principle named as holographic dark energy (HDE)
model [1]}. This principle is extensively used to study the quantum behavior of black holes.
The energy density of HDE is defined as \(\rho =3c^{2}M^{2}_{pl} L^{-2}\) , where \(c\)  is constant,
\(M_{pl}\)  plank mass and \(L\)  is supposed to be size of the universe. For the Hubble radius \(H^{-1}\) ,
this HDE model density is very similar to the observational results.
Gao et al. [2]} motivated by the holographic principle, introduced a new DE model
which is inversely proportional to Ricci scalar curvature called Ricci Dark Energy (RDE). Their
investigation shows that this RDE model solve the causality problem and the evolution of density
perturbations of matter power spectra and CMB anisotropy is not much affected by such modification.
Granda and Oliveros [3]} introduced a new infrared cut-off for the HDE model and reconstruct
the potentials and fields for different DE models such as the quintessence,
tachyon, K-essence and dilaton for FRW universe. Karami and Fehri [4]} using Granda and Oliveros
cut-off studied the non-flat FRW universe to find the DE density, the deceleration parameter and the
equation of state (EoS).
